Gravitational waves from scale-invariant vector dark matter model: probing below the neutrino-floor

Gravitational waves from scale-invariant vector dark matter model: probing below the neutrino-floor

Blog Article

Abstract We study the gravitational waves (GWs) spectrum produced during the electroweak phase transition in a scale-invariant extension of the Standard Model (SM), enlarged by a dark $$ U(1)_{D} $$ U(1)D gauge symmetry.This symmetry incorporates a vector dark matter (DM) candidate and a scalar field (scalon).Because of scale invariance, the model has only korpskaft two independent parameters and for the parameter space constrained by DM relic density, strongly first-order electroweak phase transition can take place.In this model, for a narrow part of the parameter space, DM-nucleon cross section is below the neutrino-floor limit, and therefore, it cannot be probed by the future direct detection experiments.

However, for a benchmark point from this narrow region, we show the amplitude and frequency of phase transition GW spectrum poise pads in bulk fall within the observational window of space-based GW detectors such as eLISA.